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Visualization of expanding warm dense gold and diamond heated rapidly by laser-generated ion beams
With the development of several novel heating sources, scientists can now heat a small sample isochorically above 10,000 K. Although matter at such an extreme state, known as warm dense matter, is commonly found in astrophysics (e.g., in planetary cores) as well as in high energy density physics exp...
Autores principales: | , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group
2015
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4585717/ https://www.ncbi.nlm.nih.gov/pubmed/26392208 http://dx.doi.org/10.1038/srep14318 |
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author | Bang, W. Albright, B. J. Bradley, P. A. Gautier, D. C. Palaniyappan, S. Vold, E. L. Cordoba, M. A. Santiago Hamilton, C. E. Fernández, J. C. |
author_facet | Bang, W. Albright, B. J. Bradley, P. A. Gautier, D. C. Palaniyappan, S. Vold, E. L. Cordoba, M. A. Santiago Hamilton, C. E. Fernández, J. C. |
author_sort | Bang, W. |
collection | PubMed |
description | With the development of several novel heating sources, scientists can now heat a small sample isochorically above 10,000 K. Although matter at such an extreme state, known as warm dense matter, is commonly found in astrophysics (e.g., in planetary cores) as well as in high energy density physics experiments, its properties are not well understood and are difficult to predict theoretically. This is because the approximations made to describe condensed matter or high-temperature plasmas are invalid in this intermediate regime. A sufficiently large warm dense matter sample that is uniformly heated would be ideal for these studies, but has been unavailable to date. Here we have used a beam of quasi-monoenergetic aluminum ions to heat gold and diamond foils uniformly and isochorically. For the first time, we visualized directly the expanding warm dense gold and diamond with an optical streak camera. Furthermore, we present a new technique to determine the initial temperature of these heated samples from the measured expansion speeds of gold and diamond into vacuum. We anticipate the uniformly heated solid density target will allow for direct quantitative measurements of equation-of-state, conductivity, opacity, and stopping power of warm dense matter, benefiting plasma physics, astrophysics, and nuclear physics. |
format | Online Article Text |
id | pubmed-4585717 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2015 |
publisher | Nature Publishing Group |
record_format | MEDLINE/PubMed |
spelling | pubmed-45857172015-09-29 Visualization of expanding warm dense gold and diamond heated rapidly by laser-generated ion beams Bang, W. Albright, B. J. Bradley, P. A. Gautier, D. C. Palaniyappan, S. Vold, E. L. Cordoba, M. A. Santiago Hamilton, C. E. Fernández, J. C. Sci Rep Article With the development of several novel heating sources, scientists can now heat a small sample isochorically above 10,000 K. Although matter at such an extreme state, known as warm dense matter, is commonly found in astrophysics (e.g., in planetary cores) as well as in high energy density physics experiments, its properties are not well understood and are difficult to predict theoretically. This is because the approximations made to describe condensed matter or high-temperature plasmas are invalid in this intermediate regime. A sufficiently large warm dense matter sample that is uniformly heated would be ideal for these studies, but has been unavailable to date. Here we have used a beam of quasi-monoenergetic aluminum ions to heat gold and diamond foils uniformly and isochorically. For the first time, we visualized directly the expanding warm dense gold and diamond with an optical streak camera. Furthermore, we present a new technique to determine the initial temperature of these heated samples from the measured expansion speeds of gold and diamond into vacuum. We anticipate the uniformly heated solid density target will allow for direct quantitative measurements of equation-of-state, conductivity, opacity, and stopping power of warm dense matter, benefiting plasma physics, astrophysics, and nuclear physics. Nature Publishing Group 2015-09-22 /pmc/articles/PMC4585717/ /pubmed/26392208 http://dx.doi.org/10.1038/srep14318 Text en Copyright © 2015, Macmillan Publishers Limited http://creativecommons.org/licenses/by/4.0/ This work is licensed under a Creative Commons Attribution 4.0 International License. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ |
spellingShingle | Article Bang, W. Albright, B. J. Bradley, P. A. Gautier, D. C. Palaniyappan, S. Vold, E. L. Cordoba, M. A. Santiago Hamilton, C. E. Fernández, J. C. Visualization of expanding warm dense gold and diamond heated rapidly by laser-generated ion beams |
title | Visualization of expanding warm dense gold and diamond heated rapidly by laser-generated ion beams |
title_full | Visualization of expanding warm dense gold and diamond heated rapidly by laser-generated ion beams |
title_fullStr | Visualization of expanding warm dense gold and diamond heated rapidly by laser-generated ion beams |
title_full_unstemmed | Visualization of expanding warm dense gold and diamond heated rapidly by laser-generated ion beams |
title_short | Visualization of expanding warm dense gold and diamond heated rapidly by laser-generated ion beams |
title_sort | visualization of expanding warm dense gold and diamond heated rapidly by laser-generated ion beams |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4585717/ https://www.ncbi.nlm.nih.gov/pubmed/26392208 http://dx.doi.org/10.1038/srep14318 |
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